Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications

We study the large volume limit of the scalar potential in Calabi-Yau flux compactifications of type IIB string theory. Under general circumstances there exists a limit in which the potential approaches zero from below, with an associated non-supersymmetric AdS minimum at exponentially large volume....

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Main Authors: Balasubramanian, V, Berglund, P, Conlon, J, Quevedo, F
Format: Journal article
Published: 2005
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author Balasubramanian, V
Berglund, P
Conlon, J
Quevedo, F
author_facet Balasubramanian, V
Berglund, P
Conlon, J
Quevedo, F
author_sort Balasubramanian, V
collection OXFORD
description We study the large volume limit of the scalar potential in Calabi-Yau flux compactifications of type IIB string theory. Under general circumstances there exists a limit in which the potential approaches zero from below, with an associated non-supersymmetric AdS minimum at exponentially large volume. Both this and its de Sitter uplift are tachyon-free, thereby fixing all Kahler and complex structure moduli, which has been difficult to achieve in the KKLT scenario. Also, for the class of vacua described in this paper, the gravitino mass is independent of the flux discretuum, whereas the ratio of the string scale to the 4d Planck scale is hierarchically small but flux dependent. The inclusion of alpha' corrections plays a crucial role in the structure of the potential. We illustrate these ideas through explicit computations for a particular Calabi-Yau manifold.
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spelling oxford-uuid:15998a41-abdd-4f61-a550-9dffc6ebea2e2022-03-26T10:26:25ZSystematics of Moduli Stabilisation in Calabi-Yau Flux CompactificationsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:15998a41-abdd-4f61-a550-9dffc6ebea2eSymplectic Elements at Oxford2005Balasubramanian, VBerglund, PConlon, JQuevedo, FWe study the large volume limit of the scalar potential in Calabi-Yau flux compactifications of type IIB string theory. Under general circumstances there exists a limit in which the potential approaches zero from below, with an associated non-supersymmetric AdS minimum at exponentially large volume. Both this and its de Sitter uplift are tachyon-free, thereby fixing all Kahler and complex structure moduli, which has been difficult to achieve in the KKLT scenario. Also, for the class of vacua described in this paper, the gravitino mass is independent of the flux discretuum, whereas the ratio of the string scale to the 4d Planck scale is hierarchically small but flux dependent. The inclusion of alpha' corrections plays a crucial role in the structure of the potential. We illustrate these ideas through explicit computations for a particular Calabi-Yau manifold.
spellingShingle Balasubramanian, V
Berglund, P
Conlon, J
Quevedo, F
Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications
title Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications
title_full Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications
title_fullStr Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications
title_full_unstemmed Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications
title_short Systematics of Moduli Stabilisation in Calabi-Yau Flux Compactifications
title_sort systematics of moduli stabilisation in calabi yau flux compactifications
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AT berglundp systematicsofmodulistabilisationincalabiyaufluxcompactifications
AT conlonj systematicsofmodulistabilisationincalabiyaufluxcompactifications
AT quevedof systematicsofmodulistabilisationincalabiyaufluxcompactifications